Redundancy of cosmological evolution equations in FLRW models is inevitable in general relativity and accounts for the special role of one Friedmann equation in constraining initial values.
Qualitative study of perfect-fluid Friedmann-Lemaitre- Robertson-Walker models with a cosmological constant,
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Redundancy of the cosmological evolution equations and its relationship with the initial conditions
Redundancy of cosmological evolution equations in FLRW models is inevitable in general relativity and accounts for the special role of one Friedmann equation in constraining initial values.